Geotechnical Lunar regolith simulants are developed so that engineers and researchers can explore regolith-equipment interactions ahead of deployment on the Lunar surface. A good understanding of thermo-mechanical interactions of Lunar regolith is critical to ensure the success of exploratory missions. Simulants are often evaluated based on their similarity to Lunar regolith in terms of grain-size distribution, particle shape, specific gravity, mineralogy, and chemical composition. However, the mechanical behavior of a simulant is also affected by its porosity, pore constituents, and the stress state. In this paper, the small-strain thermal and mechanical responses of two well-known commercial Lunar regolith simulants (Mare and Highland) are assessed as a function of porosity at Earth's atmospheric pressure and under vacuum. Measurements of thermal conductivity and p-wave velocity are used to monitor the impact of changes in porosity (i.e., density) and chamber pressure. The p-wave velocity data for the two simulants collapses into a single linear trendline when plotted against simulant porosity while the thermal conductivity data collapses into a single linear trendline when plotted against bulk density. Thermal conductivity is also strongly affected by chamber pressure. Thermal boundary effects make measurements conducted under 10−1 Torr inconclusive. Altogether, the results of the study provide a benchmark against which the small-strain mechanical response of other simulant candidates can be compared.
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